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Large-Scale Magnetic Field Structure at the Earth's Orbit, Its Correlation with Solar Activity and Orientation and Motion of the Solar System in the Galaxy

Published online by Cambridge University Press:  14 August 2015

G. J. Vassilyeva ,
M. A. Kuznetsova  and
L. M. Kotlyar
G. J. Vassilyeva
Affiliation:
Main Astronomical Observatory, USSR Academy of Sciences Pulkovo, Leningrad USSR
M. A. Kuznetsova
Affiliation:
Main Astronomical Observatory, USSR Academy of Sciences Pulkovo, Leningrad USSR
L. M. Kotlyar
Affiliation:
Main Astronomical Observatory, USSR Academy of Sciences Pulkovo, Leningrad USSR

Abstract

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Interplanetary magnetic field data from the different satellites obtained during the period 1963-1973 at 1 A.U. and compiled by J. King have been analysed in heliocentric ecliptic coordinates. The peculiarities of the background interplanetary magnetic field (BIMF) are discussed in relation to the orientation of the solar system in the Galaxy and the variable helioefficiency of the planets. The results of the direct cosmic experiments are evidence of the solar activity being a complex phenomenon of the solar system as a whole.

Type
Part II. Coronal and Interplanetary Responses to Long Time Scale Phenomena
Information
Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 167 - 172
Copyright
Copyright © Reidel 1980 

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